Development of a formalism for computing in situ transits of Earth-directed CMEs – Part 2: Towards a forecasting tool

Corona-Romero, Pedro; Riley, Pete

doi:https://doi.org/10.5194/angeo-38-657-2020

Articles | Volume 38, issue 3

https://doi.org/10.5194/angeo-38-657-2020

© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.

https://doi.org/10.5194/angeo-38-657-2020

© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.

Articles | Volume 38, issue 3

Regular paper

|

05 Jun 2020

Regular paper |

| 05 Jun 2020

Development of a formalism for computing in situ transits of Earth-directed CMEs – Part 2: Towards a forecasting tool

Pedro Corona-Romero and Pete Riley

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Final revised paper (published on 05 Jun 2020)
Preprint (discussion started on 02 Jan 2020)

Interactive discussion

Status: closed

AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment

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- Supplement

RC1: 'Referee report', Anonymous Referee #1, 11 Feb 2020
- AC1: 'Response Letter for Referee #1', Pedro Corona-Romero, 18 Mar 2020
RC2: 'Referee's Report', Anonymous Referee #2, 12 Feb 2020
- AC2: 'Response Letter for Referee #2', Pedro Corona-Romero, 18 Mar 2020

Peer-review completion

AR: Author's response | RR: Referee report | ED: Editor decision

ED: Publish subject to minor revisions (review by editor) (19 Mar 2020) by Peter Wurz

AR by Pedro Corona-Romero on behalf of the Authors (04 Apr 2020) Manuscript

ED: Publish as is (16 Apr 2020) by Peter Wurz

AR by Pedro Corona-Romero on behalf of the Authors (22 Apr 2020) Manuscript

Short summary

Solar storms are natural phenomena that affect technologies on which our societies are highly dependent. The understanding of solar storms and the capability to anticipate their effects on our technologies is of main interest to shield our societies. In this work we present a semi-empirical approach to increase our understanding of solar storms when they hit our planet. Additionally, we also preset a possible pathway to forecast the transits of solar storms by our planet's orbit.